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Table 2:

Two by two comparison of homogeneous sets of spectroscopic metallicities (see text).
Reference 1 Reference 2 $\Delta_{\mbox{[Fe/H]~}}$ $\sigma_{\mbox{[Fe/H]~}}$ $N_{\rm c}$ $N_{\rm o}$
Fuhrmann Mishenina 0.01 0.07 137 3
Fuhrmann Valenti -0.03 0.05 179 3
Gratton Mishenina -0.02 0.10 103 0
Gratton Ramírez 0.02 0.08 110 2
Hekker McWilliam 0.07 0.10 211 5
Luck Valenti -0.01 0.06 136 4
Mishenina Valenti -0.04 0.07 162 4
Ramírez Valenti -0.07 0.06 137 3

Notes. A simple statistic with $3\sigma$ rejection has been applied. $N_{\rm c}$ is the number of common stars, $N_{\rm o}$ is the number of $3\sigma$ outliers.


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